Abstract
Interplanetary dust particles and meteoroids mostly originate from comets and asteroids. Understanding their distribution in the Solar system, their dynamical behavior and their properties, sheds light on the current state and the dynamical behavior of the Solar system. Dust particles can endanger Earth-orbiting satellites and deep-space probes, and a good understanding of the spatial density and velocity distribution of dust and meteoroids in the Solar system is important for designing proper spacecraft shielding. The study of interplanetary dust and meteoroids provides clues to the formation of the Solar system. Particles having formed 4.5 billion years ago can survive planetary accretion and those that survived until now did not evolve significantly since then. Meteoroids and interplanetary dust can be observed by measuring the intensity and polarization of the zodiacal light, by observing meteors entering the Earth’s atmosphere, by collecting them in the upper atmosphere, polar ices and snow, and by detecting them with in-situ detectors on space probes.
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Acknowledgements
This paper was made possible by the International Space Science Institute, Bern, who brought the authors together for a whole week in 2016 and supported the meeting location and stay of the participants. All of the authors acknowledge their respective institutes and funding agencies for their support. In particular, JMTR thanks Spanish Ministry of Science and Innovation under research project AYA2015-67175-P. We acknowledge the hard work done by two referees whose comments were extremely valuable to improve this review.
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Cosmic Dust from the Laboratory to the Stars
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Koschny, D., Soja, R.H., Engrand, C. et al. Interplanetary Dust, Meteoroids, Meteors and Meteorites. Space Sci Rev 215, 34 (2019). https://doi.org/10.1007/s11214-019-0597-7
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DOI: https://doi.org/10.1007/s11214-019-0597-7